Wormholes are ECO solutions of the Einstein equations that connect different parts of the Universe or two different Universes [1]}, [2]}. Although wormholes have distinct causal strutures from BHs, they possess PSs and, therefore, can disguise themselves as BHs in GW data if one only focuses on the early stage of the ringdown signal. Lorentzian wormholes in General Relativity (GR) were discussed in [3]}, [4]}, [5]}, where a static spherically-symmetric metric was introduced and conditions for traversable wormholes were found. Unfortunately, wormhole solutions of the Einstein equations lead to the violation of null energy condition (NEC). A matter distribution of exotic or phantom matter allows the formation of traversable wormhole geometries in GR. There have been many efforts to build a wormhole with ordinary matter satisfying the NEC [5]}, [7]}, [8]} in modified gravity theories like Brans-Dicke theory [9]}, \(f({\mathcal {R}})\)  gravity [10]}, Einstein-Gauss-Bonnet theory [11]}, Einstein-Cartan theory and general scalar-tensor theories [12]}.
